SSP models for star clusters in tidal fields, based on the GALEV code
  (GALEV group webpage <http://star.herts.ac.uk/galev/>)


    Models described in: P. Anders, H.J.G.L.M. Lamers & H. Baumgardt,
    XXX XXX, XXXX (2009)



    On this page we present the SSP models for clusters evolving in a
    tidal field (and therefore changing stellar mass function).
    The time evolutions of cluster masses and magnitudes for a large
    number of filter systems are provided for
    5 metallicities ([Fe/H] = -1.7, -0.7, -0.4, 0.0, +0.4) and
    cluster dissolution timescales ranging from 100 Myr to 200 Gyr.


    This page is going to be updated regularly. New grids for other
    isochrones are on their way and will be published here soon!

The file naming conventions and formats are described in the following
README-files

 README.ps  README.txt

For further questions/requests drop me an email: p.anders /at\ uu.nl

Or visit my webpage at my current university: Utrecht university,
Netherlands <http://www.astro.uu.nl/siu/people/anders>


 


    Tarballs
    containing files with mass and magnitude evolutions for all
    available dissolution timescales.
    (If you require the integrated spectra, please contact me via email):

SSP models for z=0.0004 == [Fe/H]=-1.7 <models_z_0.0004.tgz>

SSP models for z=0.004 == [Fe/H]=-0.7 <models_z_0.004.tgz>

SSP models for z=0.008 == [Fe/H]=-0.4 <models_z_0.008.tgz>

SSP models for z=0.02 == [Fe/H]=0.0 <models_z_0.02.tgz>

SSP models for z=0.05 == [Fe/H]=+0.4 <models_z_0.05.tgz>
 
 
 


    Individual files can be found here:

 SSP models for z=0.0004 == [Fe/H]=-1.7 <models_z_0.0004/>

 SSP models for z=0.004 == [Fe/H]=-0.7 <models_z_0.004./>

 SSP models for z=0.008 == [Fe/H]=-0.4 <models_z_0.008/>

 SSP models for z=0.02 == [Fe/H]=0.0 <models_z_0.02/>

 SSP models for z=0.05 == [Fe/H]=+0.4 <models_z_0.05/>


       Some test cases (for different isochrones,IFMRs and changing-MF
      parametrisations) to estimate uncertainties <TestCases/>

Tarball of all test cases <TestCases.tgz>